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Fig. 6


Comparison between the kSZ signal and other probes of the cluster components, shown on saturated linear scales. The astrometries are the same as those in Fig. 5, and the green contours reproduce the kSZ signal-to-noise ratio, given as a solid line if positive (+2 and +3σ) and dashed line if negative (−2, −3, −4 and −5σ). Our reference regions are provided as gray circles. The positions of B1 and B2 are also shown as gray diamonds on the left image. Left: Chandra X-ray photon count image, smoothed to 7 arcsec FWHM. Middle: HST optical combined image from the CLASH data (Postman et al. 2012). Right: lensing mass (κ) from Zitrin et al. (2011).

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